This statement can be invoked to derive gravitational lensing from the entropy per wavelength of blackbody radiation. A statement similar to this one, advanced by Louis Crane, inspired Carlo Rovelli to develop a class of "relational" quantum theories. Erik Verlinde, in the context of this statement, provides a description of gravity as an entropic force. One formalism related to this statement relates the product of an anti-de Sitter space with a manifold to a conformal field theory and is also called the Maldacena duality. Its relation to the worldsheet description of string theory was outlined by Susskind. Its discoverer was motivated by finding that the bump on the event horizon of a blac
This statement can be invoked to derive gravitational lensing from the entropy per wavelength of blackbody radiation. A statement similar to this one, advanced by Louis Crane, inspired Carlo Rovelli to develop a class of "relational" quantum theories. Erik Verlinde, in the context of this statement, provides a description of gravity as an entropic force. One formalism related to this statement relates the product of an anti-de Sitter space with a manifold to a conformal field theory and is also called the Maldacena duality. Its relation to the worldsheet description of string theory was outlined by Susskind. Its discoverer was motivated by finding that the bump on the event horizon of a black hole emitting Hawking radiation has a predictable logarithmic shape. This statement was motivated by the result that a region's maximal entropy is proportional to the squared radius. For 10 points, name this statement first advanced by 't Hooft (eht HOOFT), which holds that the information in a volume of space can be encoded on its boundary.
This statement can be invoked to derive gravitational lensing from the entropy per wavelength of blackbody radiation.
{holographic principle}